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Title:
Clustering of EROs from UKIDSS DXS and Pan-STARRS PS1
Authors:
Kim, J.-W.; Edge, A. C.; Wake, D. A.; Gonzalez-Perez, V.; Baugh, C. M.; Lacey, C. G.
Affiliation:
AA(Institute for Computational Cosmology, Dept. of Physics, Durham University, Durham DH1 3LE, UK), AB(Institute for Computational Cosmology, Dept. of Physics, Durham University, Durham DH1 3LE, UK), AC(Dept. of Astronomy, Yale University, New Haven, USA), AD(Institute for Computational Cosmology, Dept. of Physics, Durham University, Durham DH1 3LE, UK), AE(Institute for Computational Cosmology, Dept. of Physics, Durham University, Durham DH1 3LE, UK), AF(Institute for Computational Cosmology, Dept. of Physics, Durham University, Durham DH1 3LE, UK)
Publication:
The Intriguing Life of Massive Galaxies, Proceedings of the International Astronomical Union, IAU Symposium, Volume 295, pp. 59-59
Publication Date:
07/2013
Origin:
CUP
Keywords:
galaxies: halos, large-scale structure, infrared: galaxies,
Abstract Copyright:
(c) 2013: Copyright © International Astronomical Union 2013
DOI:
10.1017/S1743921313004298
Bibliographic Code:
2013IAUS..295...59K

Abstract

We have measured the angular two-point correlation function of EROs. The halo model is fitted to the observed clustering, and dark matter halo mass, bias and satellite fraction are estimated in three redshift bins. We also compare our results with the semi-analytical galaxy formation model. This work illustrates the power of clustering analysis in providing observational constraints on simulations.

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